Analisis de Perturbaciones en Sistemas Interconectados de Potencia

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    By

    Mr. Richard Andrew WiltshireBachelor of Engineering

    (Electrical and Computer Engineering)1

    st Class Honours

    Doctor of Philosophy

    Centre of Energy and Resource ManagementSchool of Engineering Systems

    Faculty of Built, Environment and EngineeringQueensland University of Technology

    Brisbane, Australia.

    2007

    Analysis of Disturbances in Large

    Interconnected Power Systems

     A thesis submitted in partial fulfillment of the requirements for thedegree of 

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     Abstract

    iii

    Analysis of Disturbances in Large Interconnected PowerSystems

    by Mr. Richard Andrew Wiltshire

    Principal Supervisor:   Associate Professor Peter O’SheaSchool of Engineering Systems

    Faculty of Built, Environment and EngineeringQueensland University of Technology

     Associate Supervisor:  Professor Gerard LedwichSchool of Engineering Systems

    Faculty of Built, Environment and EngineeringQueensland University of Technology

     Associate Supervisor:  Dr Edward PalmerSchool of Engineering Systems

    Faculty of Built, Environment and EngineeringQueensland University of Technology

     

    Abstract

    World economies increasingly demand reliable and economical power

    supply and distribution. To achieve this aim the majority of power

    systems are becoming interconnected, with several power utilitiessupplying the one large network. One problem that occurs in a large

    interconnected power system is the regular occurrence of system

    disturbances which can result in the creation of intra-area oscillating

    modes. These modes can be regarded as the transient responses of the

     power system to excitation, which are generally characterised as decaying

    sinusoids. For a power system operating ideally these transient responses

    would ideally would have a “ring-down” time of 10-15 seconds.

    Sometimes equipment failures disturb the ideal operation of powersystems and oscillating modes with ring-down times greater than 15

    seconds arise. The larger settling times associated with such “poorly

    damped” modes cause substantial power flows between generation nodes,

    resulting in significant physical stresses on the power distribution system.

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     Abstract

    iv

    If these modes are not just poorly damped but “negatively damped”,

    catastrophic failures of the system can occur.

    To ensure system stability and security of large power systems, the

     potentially dangerous oscillating modes generated from disturbances

    (such as equipment failure) must be quickly identified. The power utility

    must then apply appropriate damping control strategies.

    In power system monitoring there exist two facets of critical interest. The

    first is the estimation of modal parameters for a power system in normal,

    stable, operation. The second is the rapid detection  of any substantial

    changes to this normal, stable operation (because of equipment

     breakdown for example). Most work to date has concentrated on the first

    of these two facets, i.e. on modal parameter estimation. Numerous modal

     parameter estimation techniques have been proposed and implemented,

     but all have limitations [1-13]. One of the key limitations of all existing

     parameter estimation methods is the fact that they require very long data

    records to provide accurate parameter estimates. This is a particularly

    significant problem after a sudden detrimental change in damping. One

    simply cannot afford to wait long enough to collect the large amounts of

    data required for existing parameter estimators. Motivated by this gap in

    the current body of knowledge and practice, the research reported in this

    thesis focuses heavily on rapid detection of changes (i.e. on the second

    facet mentioned above).

    This thesis reports on a number of new algorithms which can rapidly flag

    whether or not there has been a detrimental change to a stable operating

    system. It will be seen that the new algorithms enable sudden modal

    changes to be detected within quite short time frames (typically about 1

    minute), using data from power systems in normal operation.

    The new methods reported in this thesis are summarised below.

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     Abstract

    v

    The Energy Based Detector (EBD): The rationale for this method is that

    the modal disturbance energy is greater for lightly damped modes than it

    is for heavily damped modes (because the latter decay more rapidly).Sudden changes in modal energy, then, imply sudden changes in modal

    damping. Because the method relies on data from power systems in

    normal operation, the modal disturbances are random. Accordingly, the

    disturbance energy is modelled as a random process (with the parameters

    of the model being determined from the power system under

    consideration). A threshold is then set based on the statistical model. The

    energy method is very simple to implement and is computationally

    efficient. It is, however, only able to determine whether or not a suddenmodal deterioration has occurred; it cannot identify which mode has

    deteriorated. For this reason the method is particularly well suited to

    smaller interconnected power systems that involve only a single mode.

    Optimal Individual Mode Detector (OIMD): As discussed in the previous

     paragraph, the energy detector can only determine whether or not a

    change has occurred; it cannot flag which mode is responsible for the

    deterioration. The OIMD seeks to address this shortcoming. It uses

    optimal detection theory to test for sudden changes in individual modes.

    In practice, one can have an OIMD operating for all modes within a

    system, so that changes in any of the modes can be detected. Like the

    energy detector, the OIMD is based on a statistical model and a

    subsequently derived threshold test.

    The Kalman Innovation Detector (KID): This detector is an alternative to

    the OIMD. Unlike the OIMD, however, it does not explicitly monitor

    individual modes. Rather it relies on a key property of a Kalman filter,namely that the Kalman innovation (the difference between the estimated

    and observed outputs) is white as long as the Kalman filter model is valid.

    A Kalman filter model is set to represent a particular power system. If

    some event in the power system (such as equipment failure) causes a

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     Abstract

    vi

    sudden change to the power system, the Kalman model will no longer be

    valid and the innovation will no longer be white. Furthermore, if there is a

    detrimental system change, the innovation spectrum will display strong peaks in the spectrum at frequency locations associated with changes.

    Hence the innovation spectrum can be monitored to both set-off an

    “alarm” when a change occurs and to identify which modal frequency has

    given rise to the change. The threshold for alarming is based on the

    simple Chi-Squared PDF for a normalised white noise spectrum [14, 15].

    While the method can identify the mode which has deteriorated, it does

    not necessarily indicate whether there has been a frequency or damping

    change. The PPM discussed next can monitor frequency changes and socan provide some discrimination in this regard.

    The Polynomial Phase Method (PPM):  In [16] the cubic phase (CP)

    function was introduced as a tool for revealing frequency related spectral

    changes. This thesis extends the cubic phase function to a generalised

    class of polynomial phase functions which can reveal frequency related

    spectral changes in power systems. A statistical analysis of the technique

    is performed. When applied to power system analysis, the PPM can

     provide knowledge of sudden shifts in frequency through both the new

    frequency estimate and the polynomial phase coefficient information.

    This knowledge can be then cross-referenced with other detection

    methods to provide improved detection benchmarks.

    Keywords 

     Power System Monitoring, Interconnected Power Systems, Power System Disturbances, Power System Stability, Signal Processing, Optimal

     Detection Theory, Stochastic System Analysis, Kalman Filtering, Poly-

     Phase Signal Analysis.

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    Declaration

    vii

    Declaration

    I hereby certify that the work embodied in this thesis is the result of

    original research and has not been submitted for a higher degree

    at any other University or Institution.

    Richard Andrew Wiltshire

    10 July 2007

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    Table of Contents

    ix

    Table of Contents

    Abstract ............................................................................................................iii

    Keywords ......................................................................................................... vi

    Declaration ......................................................................................................vii

    Table of Contents ............................................................................................. ix

    Table of Figures .............................................................................................. xv

    List of Tables.................................................................................................. xxi

    Acknowledgements......................................................................................xxiii

    Dedication ..................................................................................................... xxv

    Glossary.......................................................................................................xxvii

    Chapter 1 ......................................................................................................... 29

    1 Introduction ............................................................................................. 29

    1.1 The Analysis of Large Interconnected Power Systems................... 29

    1.2 The Monitoring of Australia's Large Interconnected Power System.

      ……………………………………………………………………..30

    1.3 The use of Externally Sourced Simulated Data for Algorithm

    Verification ................................................................................................. 31

    1.4 Review of Existing Modal Estimation Methods ............................. 33

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    1.4.1 Single Isolated Disturbance.....................................................33

    1.4.1.1 Eigenanalysis of Disturbance Modes .................................. 33

    1.4.1.2 Spectral Analysis using Prony’s Method ............................ 34

    1.4.1.3 The Sliding Window Derivation .........................................36

    1.4.2 Continuous Random Disturbances ..........................................38

    1.4.2.1 Autocorrelation Methods..................................................... 38

    1.4.2.2 Review of Kalman Filter Innovation Strategies ..................39

    1.5 Review of Frequency Estimation Methods .....................................40

    1.5.1 Polynomial-Phase Estimation Methods................................... 41

    1.6 Conclusion.......................................................................................42

    1.7 Organisation of the remainder of the thesis.....................................43

    Chapter 2 .........................................................................................................45

    2 Rapid Detection of Deteriorating Modal Damping.................................45

    2.1 Introduction .....................................................................................45

    2.2 The Power System Model in the Quiescent State ...........................46

    2.3 The Power System Statistical Characterisation............................... 47

    2.4 PDF Verification .............................................................................50

    2.5 Setting the Threshold for Alarm...................................................... 52

    2.6 Simulated Results ............................................................................52

    2.7 Validation of Method using MudpackScripts ................................. 54

    2.8 Application to Real Data ................................................................. 56

    2.8.1 Results of Real Data Analysis .................................................58

    2.9 Discussion .......................................................................................66

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    2.10 Conclusion....................................................................................... 66

    Chapter 3 ......................................................................................................... 69

    3 Rapid Detection of Changes to Individual Modes in Multimodal Power

    Systems ........................................................................................................... 69

    3.1 Introduction..................................................................................... 69

    3.2 The Stochastic Power System Model Revisited.............................. 70

    3.3 Application of the Optimal Detection Strategy............................... 71

    3.4 Individual Mode Detection Statistic Details ................................... 73

    3.5 Statistical Characterisation of the Detection Statistic η .................. 74

    3.6 Results ............................................................................................. 77

    3.6.1 Simulated Results.................................................................... 78

    3.7 Real Data Analysis .......................................................................... 82

    3.8 Verification of Method.................................................................... 85

    3.9 Real Data Analysis Results ............................................................. 90

    3.10 Discussion ....................................................................................... 94

    3.11 Conclusion....................................................................................... 95

    Chapter 4 ......................................................................................................... 97

    4 A Kalman Filtering Approach to Rapidly Detecting Modal Changes .... 97

    4.1 Introduction..................................................................................... 97

    4.2 Stochastic Power System Model..................................................... 98

    4.3 The Kalman Application in Power System Analysis .................... 101

    4.3.1 Kalman formulation .............................................................. 101

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    4.3.2 State space representation of the power system model ......... 103

    4.3.3 Kalman Solution.................................................................... 105

    4.3.4 Detection using the Innovation..............................................106

    4.4 Simulated Data Results ................................................................. 108

    4.4.1 Simulation Type 1- damping change..................................... 111

    4.4.2 Simulation Type 2- frequency change................................... 112

    4.4.3 Simulation Type 3- damping and frequency change............. 113

    4.4.4 Statistics of results................................................................. 114

    4.5 Verification of the Kalman Method ..............................................115

    4.6 Application to Real Data ............................................................... 116

    4.6.1 Part I: Analysis of the Melbourne Data................................. 117

    4.6.2 Part II: Combining multi-site data for enhanced SNR and

    detection. ………………………………………………………………122

    4.7 Guidance in tuning the Kalman Filter ...........................................126

    4.8 Discussion on real data analysis ....................................................127

    4.9 Conclusion.....................................................................................128

    Chapter 5 .......................................................................................................129

    5 A new class of multi-linear functions for polynomial phase signal

    analysis ..........................................................................................................129

    5.1 Introduction ...................................................................................129

    5.2 The new class of multi-linear functions ........................................ 132

    5.3 Designing new GMFC members...................................................134

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    5.3.1 Algorithm for estimating the parameters of 4th order PPSs

     based on ( )31 3,T n Ω .............................................................................. 136

    5.4 Derivation of the Asymptotic Mean Squared Errors..................... 138

    5.5 Simulations.................................................................................... 145

    5.6 Application in Power System Monitoring..................................... 150

    5.6.1 Real Data Analysis and Results ............................................ 153

    5.6.2 Discussion on Real Data Analysis ........................................ 159

    5.7 Conclusion..................................................................................... 160

    Chapter 6 ....................................................................................................... 161

    6 Discussion ............................................................................................. 161

    6.1 Comparison of Proposed Detectors............................................... 166

    Chapter 7 ....................................................................................................... 175

    7 Conclusions and Future Directions ....................................................... 175

    7.1 Conclusion..................................................................................... 175

    7.2 Future Directions........................................................................... 176

    Publications ................................................................................................... 179

    Bibliography.................................................................................................. 181

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    Table of Figures

    xv

    Table of Figures

    Figure 1-1 States associated with the eastern Australian largeinterconnected power system (shaded). State capital cities thatrepresent generation nodes and measurement site location andratings are shown..............................................................................31

    Figure 2-1 Model for quasi-continuous modal disturbances in a powersystem...............................................................................................46

    Figure 2-2 Equivalent model for quasi-continuous modal oscillations in a power system....................................................................................47

    Figure 2-3 Energy PDF and Histogram Comparison (60 second window)...........................................................................................................52

    Figure 2-4 60 second Data Window of Energy Measurements with 1%False Alarm Rate Shown..................................................................53

    Figure 2-5 Mode Trajectory of QNI Case13 MudpackScript Data..........55

    Figure 2-6 Output Energy vs 1, 5, 10% thresholds..................................55

    Figure 2-7 Short Term Energy Detection Applied to Real Data, reddenotes past data used to formulate long term estimates. ................57

    Figure 2-8 24 hours of recorded angle measurements (2nd

     October 2004),sites as indicated...............................................................................59

    Figure 2-9 Queensland Estimated Impulse Response..............................59

    Figure 2-10 New South Wales Estimated Impulse Response..................60

    Figure 2-11 Victorian Estimated Impulse Response................................60

    Figure 2-12 South Australian Estimated Impulse Response....................61

    Figure 2-13 Queensland PDF Estimate with white noise verificationhistogram..........................................................................................61

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    Figure 2-14 New South Wales PDF Estimate with white noiseverification histogram. ..................................................................... 62

    Figure 2-15 Victorian PDF Estimate with white noise verificationhistogram.......................................................................................... 62

    Figure 2-16 South Australian PDF Estimate with white noise verificationhistogram.......................................................................................... 63

    Figure 2-17 Queensland 60 second energy measurements vs variousFARs shown..................................................................................... 63

    Figure 2-18 New South Wales 60 second energy measurements vsvarious FARs shown........................................................................ 64

    Figure 2-19 Victorian 60 second energy measurements vs various FARsshown. .............................................................................................. 64

    Figure 2-20 South Australian 60 second energy measurements vs variousFARs shown..................................................................................... 65

    Figure 3-1 Previously introduced stochastic power system model.......... 70

    Figure 3-2 Generation of the optimal detection statistic.......................... 72

    Figure 3-3 Mode 1 test statistic vs alarm threshold. ................................ 80

    Figure 3-4 Mode 2 test statistic vs alarm threshold. ................................ 81

    Figure 3-5 Spectral plot of mode contributions within system frequencyresponse............................................................................................ 82

    Figure 3-6 Short Term Modal Detection Applied to Real Data...............84

    Figure 3-7 Case13 Modal Damping and Frequency Trajectory. .............85

    Figure 3-8 Spectral Estimate of Site Magnitude Response. ....................86

    Figure 3-9 Estimates of Individual Modal Spectral Contributions -Brisbane (QNI).................................................................................87

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    Table of Figures

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    Figure 3-10 Estimates of Individual Modal Spectral Contributions -Sydney (NSW). ................................................................................87

    Figure 3-11 Estimates of Individual Modal Spectral Contributions -Adelaide (SA)...................................................................................88

    Figure 3-12 Individual Mode Monitoring - Mode 1 Brisbane. ................88

    Figure 3-13 Individual Mode Monitoring - Mode 1 Sydney. ..................89

    Figure 3-14 Individual Mode Monitoring - Mode 1 Adelaide.................89

    Figure 3-15 Brisbane Mode 1 Test Statistic vs Time (1% FAR).............91

    Figure 3-16 Brisbane Mode 2 Test Statistic vs Time (1% FAR).............92

    Figure 3-17 Sydney Mode 1 Test Statistic vs Time (1% FAR). ..............93

    Figure 3-18 Sydney Mode 2 Test Statistic vs Time (1% FAR). ..............93

    Figure 3-19 Magnitude spectrum of voltage angles at different sites at24:00hrs............................................................................................94

    Figure 4-1 Equivalent model for the individual response of a power

    system to load changes. ....................................................................99

    Figure 4-2 General Kalman filter estimator. ............................................99

    Figure 4-3 Innovation PSD of: a) the 60 second interval prior to thedamping change, and b) the 60 second interval subsequent to thedamping change. ............................................................................111

    Figure 4-4 Innovation PSD of: a) the 60 second interval prior to thefrequency shift, and b) the 60 second interval subsequent to thefrequency shift................................................................................112

    Figure 4-5 Innovation PSD of: a) the 60 second interval prior to thedamping change, and b) the 60 second interval subsequent to thedamping and frequency change......................................................113

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    Table of Figures

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    Figure 4-6 Analysis of Normalised Innovation prior to suddendeteriorating damping at 120mins. ................................................115

    Figure 4-7 Analysis of normalised innovation in the 60 seconds after thedeteriorating damping at 121mins. ................................................116

    Figure 4-8 Melbourne frequency response estimate from LTE at 165minutes........................................................................................... 118

    Figure 4-9 Comparison of (a) system output and (b) normalisedinnovation. .....................................................................................120

    Figure 4-10 (a) Innovation sequence γ(n), (b) Innovation PSD at 196-197mins................................................................................................121

    Figure 4-11 (a) Innovation sequence γ(n), (b) Innovation PSD at 197-198mins................................................................................................121

    Figure 4-12 (a) Innovation sequence γ(n), (b) Innovation PSD at 198-199mins................................................................................................122

    Figure 4-13 Normalised (a) Individual innovation PSDs for Sydney,Melbourne and Adelaide (b) Combination PSD at 196-197 mins.The new threshold corresponding to a 99.9% FAR....................... 125

    Figure 4-14 Normalised (a) Individual PSD at 198-199 mins (b)Combination PSD at 198-199 mins showing new threshold for CI of99.9% FAR. ...................................................................................125

    Figure 5-1 a4 estimate MSE vs. SNR for the final and intermediate parameter estimates........................................................................ 147

    Figure 5-2 a3 estimate MSE vs. SNR for the final and intermediate parameter estimates........................................................................ 148

    Figure 5-3 a2 estimate MSE vs. SNR for the final and intermediate parameter estimates........................................................................ 148

    Figure 5-4 a1 estimate MSE vs. SNR for the final and intermediate parameter estimates........................................................................ 149

    Figure 5-5 a0 estimate MSE vs. SNR for the final parameter estimates.149

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    Table of Figures

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    Figure 5-6 b0 estimate MSE vs. SNR for the final parameter estimates.........................................................................................................150

    Figure 5-7 Measured Data, (a) Voltage Magnitude and (b) Phase. .......154

    Figure 5-8 Reconstructed Signal   ( ).r  z t  ...................................................155

    Figure 5-9 Example of signal slice used for parameter estimation, down-sampled to 6.25Hz. Coloured signal shown is around the first phasedisturbance. ....................................................................................155

    Figure 5-10 Second example of signal slice used for parameterestimation, down-sampled to 6.25Hz. Coloured signal shown isaround the second phase disturbance. ............................................156

    Figure 5-11 b0 estimate. .........................................................................156

    Figure 5-12 a0 estimate (phase deg).......................................................157

    Figure 5-13 a1 estimate, 2ω π 

    = f  . ............................................................157

    Figure 5-14 a2 estimate (frequency rate), ω & . .........................................158

    Figure 5-15 a3 estimate, ω && .....................................................................158

    Figure 5-16 a4 estimate, ω &&& .....................................................................159

    Figure 6-1 EBD outputs from three sites, NSW, VIC and SA...............169

    Figure 6-2 OMID Mode 2 outputs from three sites, NSW, VIC and SA.........................................................................................................170

    Figure 6-3 OMID Mode 1 outputs from three sites, NSW, VIC and SA.........................................................................................................171

    Figure 6-4 Estimation of Spectral Mode Contributions from three sites, NSW, VIC and SA. ........................................................................172

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    List of Tables

    xxi

    List of Tables

    Table 2-1 Relative Error of Moments ......................................................51

    Table 2-2 Percentage of Alarms...............................................................54

    Table 2-3 Percentage of False Alarms over initial 3 hours of Data.........65

    Table 3-1 Qualitative Reference to Damping Performance (NEMMCO)*..........................................................................................................78

    Table 3-2 Stationary Modal Parameters and Weights..............................79

    Table 3-3 Damping Changes....................................................................80

    Table 3-4 Alarms (1% FAR) ....................................................................81

    Table 3-5 Long Term Modal Parameter Estimates ..................................85

    Table 3-6 False Alarms (1% FAR) ..........................................................91

    Table 4-1 Qualitative Reference to Damping Performance...................109

    Table 4-2 Damping and Frequency Changes to Mode 1........................110

    Table 4-3 Alarms (0.1% FAR)...............................................................114

    Table 4-4 Damping and Frequency Long Term Estimates over 120-165mins................................................................................................118

    Table 4-5 SNR Improvement through Combination of Site Analysis ...126

    Table 5-1 Approximate Formulae for CRLBs ( )1 N  >> [63].................139

    Table 5-2 Parameter Values of 4th Order Polyphase Signal used inSimulations.....................................................................................146

    Table 6-1 Comparison of detection method test statistics. ....................173

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     Acknowledgments

    xxiii

    Acknowledgements

    The author wishes to thank the following for their support during the

     period of this research. Firstly I’d like to extend a sincere thank you to

    Associate Professor Peter O’Shea, for his guidance, encouragement, input

    and patience during the period of this research. Dr O’Shea has all the

    qualities any candidate could ever ask for from a supervisor, both in his

    technical expertise and his persona, thanks Peter.

    I would also like to extend a warm thank you to Professor Gerard

    Ledwich (QUT) for his comments, guidance, input and insightful

    understanding of the research topic.

    Other people I’d like to mention and thank are Dr Ed Palmer (QUT) for

    his contributions, support and friendship over many years and Dr Chaun-

    Li Zhang (QUT) for his endless supply of data when I needed it. I would

    also like to thank Maree Farquharson (QUT) who, as fellow candidates,

    supported and encouraged each other over our respective research

     periods.

    In addition I would like to extend a grateful thank you to David Bones

    (NEMMCO) and David Vowles (University of Adelaide) for giving me

     permission to use the MudpackScripts as an important validation tool

    within this thesis, very much appreciated.

    Finally, I would like to thank the following for the much welcome

    financial support over the course of the research; Queensland University

    of Technology for the APAI and QUTPRA scholarships, the QUT

    Chancellery for providing the Vice-Chancellor’s Award, the QUT Faculty

    of Built Environment and Engineering for the BEE financial top-up and

    finally my current employer, CEA Technologies Pty. Ltd, for providing

    me the study leave I required in the final stages of completing this body

    of work.

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    Dedication

    xxv

    Dedication

    There are a number of very special people I would like to dedicate this

    work to; firstly my mother, Virginia Ann Bryan, who with her guidance,

    support and never ending devotion has helped me mature into the man I

    am today. I would also like to dedicate this work to my father, RogerWiltshire, for providing me the qualities that formulate a good engineer.

    Also to my two boys, Peter and Jack, who I am eternally proud of and

    encouraged by to strive to be a better father and person and finally to

    three very special and lovely ladies, Catherine Louise Kowalski, Meg

    Malaika (21/9/1966-19/3/2006) and Leslie Elizabeth Peters who in their

    own extraordinary way have encouraged, inspired, taught and supported

    me in my endeavours over the last few years.

    Love to you all…

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    Glossary

    xxvii

    Glossary

    AESOPS Analysis of Essentially Spontaneous Oscillations in Power Systems

    AMSE Asymptotic Mean Squared Error

    ARI Adelaide Research and Innovation

    CI Confidence Interval

    COA Centre of Area

    CRLB Cramér-Rao Lower Bounds

    CP Cubic Phase Function

    dB Decibels

    DFT Discrete Fourier Transform

    DTFT Discrete Time Fourier Transform

    EBD Energy Based Detection

    FAR False Alarm Rate

    FFT Fast Fourier Transform

    GMFC Generalized Multi-linear Function Class

    GPS Global Positioning System

    HAF Higher–Order Ambiguity Function

    HP Higher-Order Phase Function

    Hz Hertz

    IF Instantaneous Frequency

    IFR Instantaneous Frequency Rate

    IIR Infinite Impulse Response

    KID Kalman Innovation Detector

    LT Long Term

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    Glossary

    xxviii

    LTE Long Term Estimator

    ML Maximum Likelihood

    MSE Mean Squared Error

     NEMMCO National Electricity Market Management Company Limited

     NILS Non-linear Instantaneous Least Squares

     NSW New South Wales

    OIMD Optimal Individual Mode Detection

    PDF Probability Density Function

    PPM Polynomial Phase Method

    PPS Polynomial Phase Signal

    PSD Power Spectral Density

    PWVD Polynomial Wigner-Ville Distributions

    RMS (rms) Root Mean Squared

    RV Random Variable

    QLD Queensland

    QP Quartic-Phase Function

    QR Quadratic

    QUT Queensland University of Technology, Brisbane, Australia

    SA South Australia

    SNR Signal to Noise Ratio

    SVD Singular Value Decomposition

    UA The University of Adelaide

    VIC Victoria

    W Watts

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    Chapter 1

    1 Introduction

    1.1 The Analysis of Large Interconnected PowerSystems

    The worldwide economic restructuring of the electrical utility industry

    has formulated large interconnected distribution networks, resulting in a

    greater emphasis on reliable and secure operations [17]. To ensure secure

    and reliable operations, the large interconnected power systems require

    ongoing wide-area observation and control. To meet these requirements

    many wide-area monitoring methodologies have been proposed and

    established [18-20]. One of the most well accepted approaches is to

    monitor the power system at various locations within the distribution

    network and to employ Global Positioning System (GPS) information to

    synchronise the information acquired [21, 22]. With this approach, the

     positioning of the measurement locations in the network is an important

    issue which is discussed in [23].

    Monitoring of power system stability is a critical issue for distributed

    networks with a significant focus on the inter-area oscillations, whereby

    this stability is largely dependent on all “inter-area oscillations” being

     positively damped. The latter are oscillations that correspond to transient

     power flows between clusters of generators or plants within a specific

    area in the large interconnected power system [24]. Monitoring and

    control of these oscillations is vitally important, and has proven far more

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    difficult than monitoring and control of oscillations associated with a

    single generator [24].

    The inter-area oscillations (or modes) are damped sinusoids, at a given

    frequency with a relevant damping factor. It is the “ring-down” time

    associated with the damping factor that is of consequence in the transient

    ability of the system to stabilise post disturbance. It is critical that the

    transient time is short (and stable) to minimise power flows between the

    generation clusters and minimise the  associated stresses within the

    generation/transmission infrastructure. As a consequence there has been

    much work done in the area of damping factor estimation in large

    distributed power systems. Previous estimation methods have employed

    Eigen analysis [25-27] as well as Prony [28] analysis [29, 30]. For

    accurate damping factor estimation, however, one typically requires large

    amounts of data [12, 13]. Conventional damping factor estimation

    techniques are therefore not suitable for rapidly detecting sudden modal

    damping changes. This thesis addresses this shortcoming by presenting a

    variety of new monitoring methods which are able to provide indications

    of detrimental modal parameter change with short data records (typically

    of the order of minutes).

    1.2 The Monitoring of Australia's LargeInterconnected Power System.

    In Australia, the power system associated with the eastern states is an

    example of a large interconnected power system. The eastern Australian

    distribution infrastructure contains a number of generation clusters andthere are inter-area modal oscillations which arise from the interaction of

    these clusters. A generalised map of the cluster location in eastern

    Australia is shown in Figure 1-1, with the capital cities representing the

    generation nodes. Also listed in Figure 1-1 are the locations of the GPS

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    monitoring sites as presented in [22]. Due to the importance of

    monitoring inter-area oscillations, a number of partners have entered into

    collaboration to effect the monitoring. These partners include QueenslandUniversity of Technology (QUT), and various transmission distributors as

    listed in [22]. The wide-area GPS synchronised techniques outlined in

    [22] and [23] have provided the real system data analysed in this thesis.

    Queensland

    Victoria

    New South Wales

    South Australia

    Melbourne

    SydneyAdelaide

    Brisbane

    275 kV

    220 kV

    330 kV

    275 kVSouth PineBrisbane

    Para Adelaide

    RowvilleMelbourne

    Sydney WestSydney

    GPS Measurement Location& bus rating

    City

    275 kV

    220 kV

    330 kV

    275 kVSouth PineBrisbane

    Para Adelaide

    RowvilleMelbourne

    Sydney WestSydney

    GPS Measurement Location& bus rating

    City

     

    Figure 1-1 States associated with the eastern Australian large interconnected power

    system (shaded). State capital cities that represent generation nodes and

    measurement site location and ratings are shown.

    (Template image of Australia sourced from http://www.rrb.com.au/Images/Australia)

    1.3 The use of Externally Sourced Simulated Datafor Algorithm Verification

    The ultimate goal of power system monitoring algorithms is to perform

    reliably in real power system scenarios. Before this can be achieved,

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    however, the algorithms need to be tested via simulations. The simulation

    environment allows conditions to be varied and consequent performance

    to be evaluated in a controlled manner. For the simulation environment to provide useful testing, however, it must incorporate modelling which is

    representative of real systems. Good modelling strategies help to verify

    new techniques prior to real data implementation and provide confidence

    in real data analysis results. The task of creating satisfactory models of

    large dynamically interconnected systems is a challenging and non-trivial

    task. Fortunately, for the purposes of this PhD research, the author was

    given access to externally1 created simulation models and data, based on

    the eastern Australian interconnected power system. The modelling of thesystem was performed by Adelaide Research & Innovation (ARI), a

    group associated with The University of Adelaide (UA), Australia. The

    formulation of the power system model and associated data was

    commissioned and contracted by the National Electricity Market

    Management Company Limited (NEMMCO) to provide benchmark

    testing of modal estimation methods from various research centres. The

    Centre of Energy and Resource Management within the School of

    Engineering Systems at Queensland University of Technology was one of

    the research centres that was benchmark tested in 2004 [31]. The

    simulated data provided in [31] was referred to as the “ MudpackScripts”

     by the University of Adelaide authors. It consisted of various non-

    stationary data sets that were of interest in this thesis. The data set of most

    interest for this thesis is MudpackScript “Case13” which contains large

    detrimental step changes of damping. The details of the changes in the

    MudpackScripts will be presented in Chapter 2 Section 2.7 where it is

    first used for technique verification prior to real data analysis.

    1  Externally in this context means not associated with Queensland University ofTechnology, Brisbane Australia.

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    1.4 Review of Existing Modal Estimation Methods

    With power systems becoming increasingly large and interconnected, the

    resulting advantages in efficiency have been offset somewhat by thedisadvantage of greater vulnerability to system instability. This latter

     problem has made it very important to be able to perform reliable

    detection of system disturbances from modal oscillation data records.

    These data records can be associated with either a single isolated

    disturbance or with continuous random disturbances. The power

    industry’s chief concern is in the detection of exponentially growing

    disturbance modes potentially present in the power system. If a growing

    mode is detected then the power utilities must introduce some dampening

    to counteract the mode. As a result, methods for fast, reliable and accurate

    estimation of the modal parameters are very important.

    1.4.1 Single Isolated Disturbance

    The parameter estimation methods in this section of the literature review

    focus on the power system’s response to a single isolated disturbance.

    1.4.1.1 Eigenanalysis of Disturbance Modes

    There are a number of well established methods that have been used for

    the analysis of power systems. Many of these methods assume that the

    intrinsically non-linear power system can be approximated as a linear

    system for small perturbations from the steady state. Under this

    assumption Kundur et. al . [32] showed that eigenvalue analysis

    techniques could be quite effective. Conventionally, eigenanalysis of a

     power system is carried out by explicitly forming the system matrix, then

    using the standard QR algorithm to compute the eigenvalues of the matrix

    [32]. Modal oscillation parameters were then obtained from the

    eigenvalues. This basic method has proven to be generally reliable and

    has been extensively used by power utilities worldwide. Unfortunately

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    this method is unsuitable for large interconnected systems [26]. To enable

    large system mode monitoring the basic Eigen methods above have

    undergone various adaptations. Byerly et. al.  [7] developed the best-known algorithm – AESOPS (Analysis of Essentially Spontaneous

    Oscillations in Power Systems). The advantage of AESOPS is that it does

    not require the explicit formation of the system state matrix [7]. The

    shortfall of the AESOPS method is the inadequacy for analysing very

    large interconnected systems.

    Uchida and Nagao [25] made another development in eigenanalysis by

     proposing the use of the “ S   matrix method”. In this method, it is

    assumed that the dynamics of power systems can be linearly

    approximated with a set of differential equations of the form,  Ax=& ,

    where is the (vector) state of the system and  A   is the system matrix.

    The S   matrix method transforms the matrix, A , into the matrix,

    1( )( )S A hI A hI    −= + − , where  I  is the unit matrix and h  is a positive real

    number. It can be shown that the dominant eigenvalues of S  are the same

    as the dominant eigenvalues of  A , but with an appropriate choice for h,

    can be computed with better numerical precision and speed [25]. The

    refined Lanczos process is also employed to make high-speed calculation

     possible [25]. Despite the computational advantage of the “ S   matrix

    method” eigenanalysis has limited application for very large

    interconnected power systems [33].

    1.4.1.2 Spectral Analysis using Prony’s Method

    The spectral analysis of modal parameters for power system disturbance

    monitoring is another area of research which has received much attention.

    In this approach power system disturbance data records are spectrally

    analysed immediately after a fault or disturbance. One popular technique

    used for the spectral analysis is Prony’s method, which originated in an

    earlier century [28]. Its ability to be practically implemented, though, was

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    delayed until the advent of the digital computer. Numerical conditioning

    enhancements developed in 1982 by Kumaresan and Tufts [3] broadened

    its applicability to modal estimation. C.E Grund et. al.  [33] comparedProny analysis to eigenanalysis and stated that “ Prony analysis has an

    important advantage over eigenanalysis techniques in that it does not

    require the derivation of a medium-scale model ”. Additionally, it can also

     be applied to field measurements for the derivation of control design

    models [33]. Many papers have been written on the use of Prony analysis

    for oscillation modal parameter estimation [34], [29] , [35], with each

     providing its own insights.

    It should be noted however that the above applications of Prony’s method

    assume that the signal contains little noise. In practice methods based on

    the Prony technique are only effective where the noise power is relatively

    small. Trudnowski et. al. [30] alluded to this when they stated for Prony

    analysis “…The accuracy of the mode estimates is limited by the noise

    content always found in field measured signals…”.

    The poor conditioning of Prony’s method exists because of an ill-

    conditioned matrix inversion in the method. To improve the ill

    conditioning, Kumaresan and Tufts [3] [4] proposed using a “Pseudo-

    Inverse” matrix, incorporating Singular Value Decomposition (SVD).

    This technique was further explored by Kumaresan and Tufts in [4] and

    was an improvement of the backward linear prediction methods proposed

     by Nuttall [36], which in turn were improvements of Prony’s original

    method.

    This process of applying a truncated SVD analysis effectively increases

    the SNR in the data prior to obtaining the solution vector. In [3],

    simulations show that this method gives much more accurate estimates of

    the modal parameters than traditional Prony methods. In [2], Kumaresan

    also provided further enhancement to Prony’s method with the

    introduction of FIR pre-filtering to reduce the sensitivity of measurement

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    errors in observed signal samples when determining the parameters of

    sinusoidal signals.

    Gomez Martin and Carrion Perez also introduced some extensions in

    working with noisy data with the application of Prony’s method [6] by

    using a moving window in both forward and backward directions. This

    application of forward and backward methodologies were further

    explored by Kannan and Kundu [37].

    A time-varying Prony method for instantaneous frequency estimation

    from low SNR data was introduced by Beex and Shan [38]. This was

     pertinent since power systems do have substantially non-stationary

    components on occasions. 

    1.4.1.3 The Sliding Window Derivation

    Prony’s method is a parametric spectral analysis method. Some authors

    have pursued solutions using classical spectral analysis based on Fourier

    methods. For example; Poon and Lee [39] developed a technique to

    determine the modal parameters by employing a Sliding Window Fourier

    Transform. The frequency components of the modes were first identified

    in the frequency spectrum. The damping constants could then be obtained

     by comparing the spectral magnitudes of a given modal component in

    different time windows. These Fourier techniques proved to be quite

    robust to noise and worked well as long as the oscillation modes were

    well separated and could be separately distinguished within the Fourier

    spectral domain.

    Basically the method developed by Poon and Lee uses the rate of decay

    of the Fourier Transform as a rectangular window slides to determine thedamping factor of the mode. The results of this method provided good

    correlation compared to conventional techniques. However the

    fundamental limitation of the Poon and Lee method was the tight

    restrictions on the length of the window that could be used.

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    It was subsequently shown that this restriction was needed to avoid errors

    due to the interference from the superposition of the positive and negative

    frequency components [9]. This interference was formulated by the largeside lobes of the spectral  sinc  function introduced by the rectangular

    windowing. Hence, Poon and Lee specified that the window lengths only

    have certain discrete values, at which the interference (zeros in the  sinc 

    function) turned out to be zero. The problem was that the window length

    was dependent upon the modal frequency, and hence this frequency had

    to be accurately estimated prior to the windowing implementation.

    Additionally, a different set of windows was required to process every

    different mode present. O’Shea [8] extended Poon and Lee’s Fouriermethod and showed that a relaxation of the restriction on window lengths

    could be achieved by applying a smooth tapering window (Kaiser

    window) rather than a rectangular one [40], [9].

    Although the sliding spectral window methods in [39] and [9] were robust

    to noise, they only allowed analysis of multiple modes if the modes were

    sufficiently well separated to be resolved with conventional Fourier

    techniques. To deal with multiple closely spaced modes Poon and Lee

    [41] developed a modified technique. For lightly damped closely spaced

    low frequency oscillation modes exhibiting beat phenomenon they made

    use of the imaginary part of the Fourier Transform of the swing curves.

    Their simple dual modal case was modelled by:

    1 2

    1 1 2 2( ) cos(2 ) cos(2 )t t  f t a f t e a f t eσ σ π π − −= +

      (1.1)

    and 1 f   and 2 f   were assumed to be close in frequency and unable to be

    resolved using Fourier techniques.

    Although not specifically stated by Poon and Lee, a major problem with

    their method was that it was not straightforward to determine either 1 f   or

    2 f  . It was therefore not straightforward to determine the damping factors.

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    O’Shea [42] showed that a simpler and more reliable method of

    determining modal parameters for closely spaced modes was to extend

    the earlier Sliding Window method in [9] by calculating the spectrum inmore than two windows. Using the results from the multiple spectral

    windows, a set of simultaneous equations in the desired parameters could

     be created. These parameters were the complex amplitudes, frequencies

    and damping factors of the modes. These simultaneous equations could

    then be solved in a least squares sense [4] to obtain estimates for the

    modal parameters. The presented simulations indicated good results.

    1.4.2 Continuous Random Disturbances

    The methods for modal analysis so far discussed all assumed that the data

    record could be well modelled as a sum of complex exponential modes.

    This is an acceptable model if the record has been obtained after a single

    isolated disturbance. However this is not acceptable for a record obtained

    from continuous random disturbances (which is the scenario for power

    systems in normal operation [11]). The following sections investigate

    modal parameter analysis in relation to continuous random disturbances.

    1.4.2.1 Autocorrelation Methods

    The estimation of modal parameters from data records corresponding to

    continuous random disturbances was discussed by Ledwich and Palmer in

    [11]. They reasoned that the continuous random disturbances exciting a

     power system in normal operation should be fractal in nature, having a 1/ f  

    shaped spectrum [11], i.e. it should be equivalent to integrated white

    noise. They also reasoned that a power system could be approximated as

    an IIR filter. With these assumptions about the excitation and power

    system, Ledwich and Palmer showed that if one differentiated the output

    of the power system, the result would be equivalent to the output of an

    IIR filter driven by white noise. Since the autocorrelation function of a

    system driven by white noise reveals the impulse response of that system

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    [43], then the autocorrelation function of the differentiated power system

    disturbance output should be the impulse response of the power system,

    i.e. it will have the form of a sum of complex exponentials. The modal parameters can then be determined using Prony analysis [11].

    Autocorrelation techniques were further examined by Banejad and

    Ledwich [12] to determine resonant frequencies and mode shape by

    modelling disturbances using white noise to represent customer load

    variations and an impulse to represent a disturbance. The simulation

    results provided tangible relationships to a known system’s eigenvalue,

    resonant frequencies and mode shape, but did not make any reference to

    the limitations of mode spacing.

    1.4.2.2 Review of Kalman Filter Innovation Strategies

    In the 1950s, increased control requirements for advancing avionics led to

    the formulation of what is now commonly known as the Kalman filter.

    Although earlier radar tracking work by Swerling had formulated very

    similar algorithms [44] the more highly recognised publications by

    Kalman [45], [46] then Kalman and Bucy [47] were generally recognised

    as the origins of the Kalman filter. Since that time the Kalman filter has

     been recognised as a very important (and optimal) linear estimator; it has

     been used extensively in a multitude of areas that encompass stochastic

    models, state and parameter estimation and control requirements. There

    have also been a multitude of Kalman filter variations for non-linear

    systems, such as the extended Kalman filter [48] and unscented Kalman

    filter [49]. In this thesis, the focus of interest is on the Kalman filter

    innovation. The innovation is defined as the difference between the

    measured output and the estimated output [50]. It is well known that the

    innovation from a Kalman filter is spectrally white as long as the assumed

    model parameters are valid [50, 51]. However under faulty or changed

    conditions the innovation sequence will demonstrate large systematic

    trends as the model will no longer represent the physical system [50].

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    Various Kalman filter innovation approaches, that target fault detection,

    diagnosis of dynamic systems and least squares estimation, are presented

    in [50-55]. In this thesis the Kalman filter model is used to estimate thesystem output. By monitoring the whiteness of the innovation one can

    detect if there are any sudden detrimental changes in the model

     parameters [50], otherwise the innovation sequence is equivalent to the

    original excitation under normal plant conditions [51].

    1.5 Review of Frequency Estimation Methods

    Although modal damping estimates are of critical importance, the

    frequency of the modes also provides an opportunity to determine

    changes in system behaviour and dynamics. In the case of large

    interconnected power systems, if a particular major site disconnects from

    a national grid (example South Australia disconnects from the Australian

    Eastern network) then the resulting power system will undergo a dynamic

    shift in an attempt to re-establish an equilibrium state. In doing so it is

    expected that the frequencies of the remaining modes will also change.

    Therefore to rapidly detect and estimate the changes in modal frequencies

    is of critical importance.

    The nature of the frequency changes that occur in a power system over

    time will not be known precisely. To allow for the arbitrary nature of the

    frequency trajectories, polynomial modelling will be used. Note that if the

    frequency trajectory is a polynomial as a function of time, then the phase

    trajectory will also be polynomial. It will be assumed that the

    component/mode in question is given by:

    ( ) ( )0( ) , j nr w z n b e z nφ = +  (1.2)

    where b0 is the amplitude, the polynomial phase coefficients are given by

    { }0 1, , ,  P a a aK  and the phase is:

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    0

    ( ) P 

     p p

     p

    n a nφ =

    = ∑  (1.3)

    and ( )w z n  is complex white Gaussian noise.

    1.5.1 Polynomial-Phase Estimation Methods

    To determine the frequency/phase trajectory of a component/mode

    conforming to the model in (1.2) it is necessary to determine the

     polynomial phase coefficients. An obvious solution to the problem of

    obtaining estimates of these parameters is to use the direct Maximum

    Likelihood (ML) method. However as discussed in [56] the

    implementation of this method is very computationally intensive,

    requiring a  P -dimensional search. To overcome the computationally

    restrictive implementation of the ML method, various authors have

    introduced alternative strategies [57], [58], [59], [60] and [61].

    Fundamentally these strategies employ multi-linear transforms that

    reduce the search requirements from a P -dimensional search to a far more

    computationally efficient P -one-dimensional search.

    More recently O’Shea introduced a “time-frequency rate” representation

    which is defined in equation (1.4) [16]:

    ( )( )

    ( )2

    1 / 2

    0

    ( , ) .r 

     N  j m

     z r r m

    CP n z n m z n m e−

    − Ω

    =Ω = + −∑

      (1.4)

    This representation reveals the rate of change of frequency of a signal as a

    function of time. This has some relevance to the power system scenario

    where frequency changes are of particular interest. If n is set equal to 0 in

    equation (1.4) the Cubic Phase (CP) function is obtained. This function

    has been demonstrated to be very effective in the estimation of

    Polynomial Phase Signals (PPS) up to orders of   3 P  = . The

    computationally efficient implementation of the CP was procedurally

    outlined by O’Shea in [62]. This fast algorithm was shown to produce

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     predictable estimate Mean Squared Errors (MSE) in close proximity to

    relevant Cramér-Rao Lower Bounds (CRLBs), above a given Signal to

     Noise Ratio (SNR) threshold. The relevant CRLBs associated with thePolynomial Phase Coefficients for a given order PPS are outlined in [63].

    Generalised higher order (HP) phase functions were also introduced by

    O’Shea in [62]. The HP function formed a multi-linear extension to the

    CP function, specifically for the purposes of parameter estimation of PPS

    of order greater than three. The definition of this function is shown below

    in (1.5),

    ( )

    2

    ( , ) , ,r r 

     P P j m

     z z m

     HP n K n m e− ΩΩ =∑   (1.5)

    where ( )   ( ) ( )1,i

    i i

    r k k  P I 

     z i r i r i K n m z n c m z n c m∗

    =  = Π + −

     

    is the kernel and [ ] 

    . ir ∗

     indicates conjugation of [ ]. iff   1ir  = .

    The parameters , ,i ic k  , andir I  are selected to ensure unbiased parameter

    estimates for a phase polynomial of order  P . The choice of these

     parameters was conducted in a comparable manner to procedures outlined

    in [61] and [59], to ensure unbiased phase coefficient estimates.

    Further work on the HP function was explored by Farquharson et. al.  in

    [56]. New HP functions were devised that allowed parameters to be

    determined in isolation [56]. It was noted in [56] that the new HP

    functions had some similarities to functions introduced in [60], but they

    also had some notable differences. In particular the new HP function

     based estimates in [56] had much lower SNR thresholds and were

    therefore much more practically applicable.

    1.6 Conclusion

    Despite the advances of the last decades for modal parameter estimation

    techniques, there is a common recognition by many authors that no

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    individual technique accounts for all the various situations that arise in

     practice. Each tool has its own merits and applications, and provides a

    different view into dynamic system behaviour. With technologicaladvances constantly changing the face of power systems, the need to

    continually improve oscillation modal estimation algorithms has been

    widely accepted as being very important. Reliable detection of sudden

    detrimental changes in modal oscillations is also extremely important so

    that catastrophic failures can be avoided. Relatively little work has been

    done to date on optimal procedures for such detection.

    In relation to frequency and frequency rate estimates methods outlined

    earlier, it is important to keep in mind the desire of the power industry to

    obtain estimates as quickly as possible with an acceptable level of error.

    In the situation of angle measurements from sites around a national power

    system, it is generally recognised that these recorded measurements have

    a reasonable SNR. These SNRs should be adequate for the PPS modelling

    approaches considered in this thesis for estimating/detecting changes in

     post-separation modal frequencies.

    Therefore the major focus of this thesis will be the rapid acquisition of

    system information (both modal damping and modal frequency) under the

    scenario of sudden detrimental change to a quasi-stationary large

    interconnected power system.

    1.7 Organisation of the remainder of the thesis

    The remainder of the thesis is organised as follows. Chapter 2 introduces

    a unique energy based method that is primarily focused on the rapid

    detection of deteriorating modal damping in power systems. In Chapter 3 

    the technique in Chapter 2  is further extended and optimised for

    monitoring of individual modal damping changes in multi-modal power

    systems. Chapter 4  will then introduce another prospect of modal

     parameter monitoring which is based around the Kalman filter innovation

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    spectrum. Chapter 5 will introduce a new class of multi-linear functions

    for polynomial phase signal analysis and examine implementation

    opportunities in power system monitoring. Chapter 6  will be devoted to ageneral discussion and Chapter 7   will present conclusions and future

    directions.

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    Chapter 2

    2 Rapid Detection of Deteriorating ModalDamping

    2.1 Introduction

    In this chapter a new method is introduced that deals with the problem of

    detecting sudden changes in the damping of inter-area modes in large

    interconnected power systems. The motivation for focus on rapid

    detection, rather than the more traditional modal parameter estimation, is

    drawn from the verity that standard modal parameter estimation methods

    require long data records to yield accurate estimates – typically an hour or

    more of data is needed. This is too long to wait if there is a sudden andseriously problematical change of damping.

    While accurate estimation of the modes requires long time scales,

    detection of sudden deterioration from a known quiescent point can be

    done in much shorter time scales (typically a minute). The “sudden

    change” can be detected very easily via a sudden change in the energy of

    the system modes. However to be able to make an informed decision on

    whether a change has actually occurred a statistical characterisation of the

    quiescent system energy must be established. Once the statistical

    characterisation has been formulated the thresholds for rapid detection of

    modal deterioration may be set that can provide an alarm benchmark with

    a defined confidence level.

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    ideally obtained according to the procedure in [23]. This procedure

    maximises the lightly damped inter-area mode information and minimises

    the effect of the more heavily damped local modes (that are less critical inregards to overall supply stability and control).

    Power System Filter 

    h(n)Integrator 

    white noise,

    w(n)γ(n)

    Differentiate

     y(n)

    Power System Filter h(n)

    white noise

    w(n) y(n)

    output 

     x(n)Power System Filter 

    h(n)Integrator 

    white noise,

    w(n)γ(n)

    Differentiate

     y(n)

    Power System Filter h(n)

    white noise

    w(n) y(n)

    output 

     x(n)

     

    Figure 2-2 Equivalent model for quasi-continuous modal oscillations in a power

    system.

    With the power system model established, a statistical characterisation of

    the system energy will be formulated in the following section.

    2.3 The Power System Statistical Characterisation

    The rationale behind the method proposed in this chapter is that the

    energy of the output,  y(n), will remain stable unless either the power

    system filter transfer function or the excitation noise level changes

    suddenly. If the power system transfer function changes such that there is

    less damping of the excitation noise, then the result is more energy within

    the output signal. Alternatively if there is a sudden (and sustained)

    increase in excitation energy there could be a fault. In either case an

    alarm should be created so that appropriate investigation/control can be

    implemented.

    This section will apply the knowledge of the power system model

    established in [11] to generate a statistical system characterisation. A

    formula is derived for a probability density function (PDF) of the energy

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     y(n)  under quasi-stationary operating conditions. The statistical

    characterisation of the energy y(n) enables a reliable threshold to be set so

    alarms can be raised if the energy deviates too much from these quasi-stationary operating conditions.  These operating conditions can be

    determined by the types of techniques described in [11]. As the detection

    condition is for large detrimental change then the False Alarm Rate

    (FAR) for detection is usually set fairly low (1% or lower). Such a low

    FAR facilitates the minimisation of unwanted false alarms. Once an alarm

    has been triggered, further monitoring of the system energy is necessary.

    Sequential data windows are collected and a statistical analysis with

    respect to the PDF is undertaken. Repeated alarms due to consistentlyhigh energy readings would induce corrective action by the power system

    utility.

    To develop the PDF for the energy in  y(n)  we return to the model in

    Figure 2-2. It follows from Figure 2-2 that the output signal’s discrete

    Fourier transform is:

    ( ) ( ) ( ),Y k H k W k  =   (2.1)

    where  H(k)  is the discrete Fourier transform (DFT) of h(n), W(k)  is the

    DFT of w(n) and Y(k)  is the DFT of  y(n). Now, according to Parseval’s

    theorem, the energy of y(n) can be determined from the samples in either

    the time domain or the frequency domain. Because the samples are

    independent in the frequency domain, though, this domain is most

    conducive to developing a statistical characterisation. Note also, that for

    real signals, all the information in the frequency domain is contained in

    the positive half of the spectrum – the information in the negative half is

     just a copy of that contained in the positive half. Using Parseval’s

    theorem and the fact that half the energy is contained in the positive half

    of the spectrum for real signals, total energy of y(n) is:

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    }|)0(||)0(|2

    1|)(||)({|

    2 222/

    1

    22W  H k W k  H 

     N  E 

     N 

    ∑=

    +=   (2.2)

     Note that ( )W k    is a complex Random Variable (RV) with real and

    imaginary parts:

    ( ) ( ){ }   ( ){ }2 2 2

    Re ImW k W k W k  = +   (2.3)

     Now if the variance of w(n) is 2σ  , then the left hand side of (2.3) is a chi-

    squared RV with two degrees of freedom and variance, N 

    2σ    [15].

    Therefore the PDF at any discrete ensemble frequency ik   is:

    ( ){ } 22 2 , xN 

    i

     N  f W k e   σ 

    σ 

    =   (2.4)

    where x is the random variable power.

    Using (2.1) and (2.4) the PDF of ( )ik Y   can be deduced to be:

    ( )

    ( )

    ( )2 2

    2 2

    2 2

    ( ) ( )

    .

    i

    i

     y k w

    i i

     N 

     H k  x

    i

     x f Y f 

     H k H k 

     N e

     H k 

    σ 

    σ 

    =

    =

      (2.5)

    From (2.2) it is evident that the energy is obtained by summing / 2 1 N    +  

    RVs and then scaling by 2/N . Furthermore these RVs have PDFs given by

    (2.5). The PDF of the sum is obtained by convolving the PDFs of all the

    RVs being summed. That is, the PDF of this sum is:

    ( )   ( ) ( ) ( )/ 2 / 2 1 0/ 2 / 2 1 0 N N  y y N y N y

     f x f x f x f x−   −= ∗ ∗ ∗L   (2.6)

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    ( )   ( )

    ( )   ( )

    ( )   ( )

    2 212

    2 2

    2 2

    2 012

    2 1

    2

    2 / 2

    0

    1 ,

    / 2

     xN H 

     xN H 

     xN H N 

     H e

     N  H e

     H N e

    σ 

    σ 

    σ σ 

    − −

    − −

    − −

    −   −

    −   −

    −   −

    = ∗

    ∗ ∗ L

      (2.7)

    where * denotes convolution.

    Finally the PDF of the energy is obtained from the sum by scaling by 2/N .

    The final energy PDF must therefore have its axes re-scaled accordingly.

    From the PDF the threshold for detection of change can be formulated.

    Establishing say the 1% false alarm rate is obtained via the cumulative

    summation of the PDF area until the 99% point is determined.

    2.4 PDF Verification

    To verify the theoretically determined system output PDF, a comparison

    of a theoretical PDF and simulated histogram was undertaken. Using

    known modal parameters, simulations created a collection database of

    outputs that were formulated into a histogram. A theoretical PDF was

    then formulated and compared directly to the histogram. 

    The procedure for verification involved 10,000 simulation runs of random

    noise,   ( )~ 0,1 N  , feeding a known modal system, depicted in Figure 2-2

    and defined below:

    ( ) ( ) ( )1 2 ,h n h n h n= +   (2.8)

    where

    ( )   ( )sin 1,2ini i i ih n A e n iσ  ω φ −= + =   (2.9)

    with modal parameters:

    11 1 1 11.7 / , 0.4 , 1, 0r s s Aω σ φ 

    −= = − = =   o  

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    12 2 2 22.7 / , 0.52 , 1, 0r s s Aω σ φ 

    −= = − = =   o  

    Energy measurements were based on a 20, 40 and 60 second data window

    with a sampling rate of 5Hz. Statistical characteristics of the simulated

    histogram and of the theoretical PDF were calculated and compared. The

    statistical characteristics examined were the first three central moments,

    mean, variance and skewness [64]. The percentage errors between the

    theoretical and simulated PDFs are shown in Table 2-1. The errors are all

    comparatively low, inspiring confidence in the fact that the derived PDF

    is correct.

    TABLE 2-1 R ELATIVE ERROR OF MOMENTS 

    TIME WINDOW  20SEC  40SEC  60SEC 

     NOISE VARIANCE  1.0 1.0 1.0

    MEAN  0.04% 0.43% 1.67%

    VARIANCE  0.82% 1.65% 0.24%% 

    ERROR  

    SKEWNESS[64] 2.59% 5.76% 6.53%

    Further validation of the theoretical PDF is provided by a visual

    comparison with a histogram. The result from a 60sec analysis window is

    shown in Figure 2-3. There is a close visual alignment.

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    5 10 15 20 25

    0

    10

    20

    30

    40

    50

    60

    70

    80

    Output half energy hisogram vs PDF

    Energy-Joules

    Output Energy Histogram vs PDF

    5 10 15 20 25

    0

    10

    20

    30

    40

    50

    60

    70

    80

    Output half energy hisogram vs PDF

    Energy-Joules

    Output Energy Histogram vs PDF

     

    Figure 2-3 Energy PDF and Histogram Comparison (60 second window).

    2.5 Setting the Threshold for Alarm

    From the PDF the threshold for detection of change can be formulated.

    Establishing say the 10% false alarm rate is via the cumulative

    summation of the PDF area until the 90% point is determined.

    2.6 Simulated Results

    It will be seen in this section that the simulations for detecting change

     provided good results. The modal values were initially set to:

    Mode 1: ( )0.4 sin 2t e t −   1 0.4σ ∴ = − 1& 2.0 /r sω   =  

    Mode 2: ( )0.52 sin 2.7t e t −   2 0.52σ ∴ = − 2& 2.7 /r sω   =  

    In the 300 minutes of simulated data, mode 1 underwent two damping

    changes; a step deterioration to 1 0.1σ   = −   damping at 100 mins and

    another step change to 1 0.2σ   = −  damping at 200 mins. The variance of

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    the driving noise, w(n), was set to unity. The output,  y(n), was generated

    as per the model shown in Figure 2-2. Energy measurements for the

    output were then taken over 1 minute block periods. The first 100 minutesrepresent the quasi-stationary system prior to the damping changes.

    The graphical results and relevant statistics are shown in Figure 2-4 and

    Table 2-2 respectively. The results are as one would expect – a low alarm

    rate for the quiescent conditions, a high alarm rate during the major

    damping change, and a lesser alarm rate during the period when the

    damping “corrects itself” somewhat.

    0 50 100 150 200 250 3000

    10

    20

    30

    40

    50

    60

    70

    Half Output Energy vs Time

    Time-Minutes

       E  n  e  r  g  y  -   J  o  u   l  e  s

    Energy

    1% FAR

    Output Energy vs Time

    0 50 100 150 200 250 3000

    10

    20

    30

    40

    50

    60

    70

    Half Output Energy vs Time

    Time-Minutes

       E  n  e  r  g  y  -   J  o  u   l  e  s

    Energy

    1% FAR

    Output Energy vs Time

     

    Figure 2-4 60 second Data Window of Energy Measurements with 1% False Alarm

    Rate Shown.

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    TABLE 2-2 PERCENTAGE OF ALARMS 

    FALSE ALARM R ATE SET AT 1%

    0-100 MIN  NO CHANGE 

    11 4.0

      −−=  sσ   

    100-200 MIN 

    STEP CHANGE 1

    1 1.0  −−=  sσ   

    200-300 MIN STEP CHANGE 

    11 2.0

      −−=  sσ   

    % OF TIMEALARM O N 

    0.0% 80.0% 32.0%

    2.7 Validation of Method using MudpackScripts

    In this section the energy based method is verified using the Case13

    MudpackScript data.

    This data set is useful as it contains an initial 2 hour section that may be

    regarded as representing the power system in a quasi-stationary state with

    acceptable damping. It is this initial 2 hour section that is analysed by the

    LTE to generate the required system PDF. From this the desired threshold

    can be set. This data set used for verification represents the Queensland

    (QNI) mode of the power system. Within this QNI data, the damping

    suddenly deteriorates from an acceptable -0.25 to a very

    undesirable 0.05− . The trajectory of the damping factor associated with

    the Case13 script can be seen in Figure 2-5.

    The detection results from the analysis of the first 12 hours of data can be

    seen in Figure 2-6. The analysis window used is a block window set to 60

    seconds at a 5Hz sampling rate. Comparison of Figure 2-5 and Figure 2-6

    shows that the energy experiences sudden jumps when the damping

    experiences sudden jumps, as one would hope. Various different alarm

    thresholds are shown in Figure 2-6; for the data under analysis it is seen

    that if one uses a 1% false alarm rate, one only gets alarms when there are

    genuine damping changes.

    In the following section, the energy detection technique will be applied to

    real multi-site data obtained from wide area monitoring sites.

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    2 4 6 8 10 12

    -0.3

    -0.25

    -0.2

    -0.15

    -0.1

    -0.05

    0

    Time-hrs

       D  a  m  p   i  n  g

    MudpackScript Case13 QNI Damping Trajectory

     

    Figure 2-5 Mode Trajectory of QNI Case13 MudpackScript Data.

    0 2 4 6 8 10 120

    1

    2

    3

    4

    5

    6

    7

    x 10-3 Output Energy vs Time

    Time-hrs

       E  n  e  r  g  y  -   J  o  u   l  e  s

     

    Energy

    10% FAR

    5% FAR

    1% FAR

     

    Figure 2-6 Output Energy vs 1, 5, 10% thresholds.

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    2.8 Application to Real Data

    To apply the energy detection method to a real data situation a long term

    estimator is required to provide an estimation of the quiescent modalvalues. Initially the long term estimator establishes estimates for the

    system transfer function. From this an estimated impulse response can be

    determined. With this knowledge an approximation of the variance of the

    excitation signal, w(n)  in Figure 2-1, can be estimated. Once the system

    transfer function, h(n), and the excitation variance, 2σ  , have been

    estimated then the expected energy PDF can be formulated. It is this

    formulated PDF that enables a threshold to be set (given a suitable false

    alarm rate). Note that the long-term estimate is periodically updated, and

    the threshold is changed, based on the updated estimate.

    The process for simultaneously performing the long-term estimation,

    generating the energy estimate, thresholding and alarming is depicted

    diagrammatically in Figure 2-7. As shown in Figure 2-7, the first task is